The University of Southampton
University of Southampton Institutional Repository

Polycyclic aromatic hydrocarbon emission in the central regions of three Seyferts and the implication for underlying feedback mechanisms

Polycyclic aromatic hydrocarbon emission in the central regions of three Seyferts and the implication for underlying feedback mechanisms
Polycyclic aromatic hydrocarbon emission in the central regions of three Seyferts and the implication for underlying feedback mechanisms

We analyze JWST Mid-Infrared Instrument/Medium Resolution Spectrograph integral field unit observations of three Seyferts from the Galactic Activity, Torus, and Outflow Survey (GATOS) and showcase the intriguing polycyclic aromatic hydrocarbon (PAH) and emission-line characteristics in regions of ∼500 pc scales over or around their active galactic nuclei (AGN). Combing the measurements and model predictions, we find that the central regions containing a high fraction of neutral PAHs with small sizes, e.g., those in ESO137-G034, are in highly heated environments, due to collisional shock heating, with hard and moderately intense radiation fields. Such environments are proposed to result in inhibited growth or preferential erosion of PAHs, decreasing their average size and overall abundance. We additionally find that the central regions containing a high fraction of ionized PAHs with large sizes, e.g., those in MCG-05-23-016, are likely experiencing severe photoionization because of the radiative effects from the radiative shock precursor besides the AGN. The severe photoionization can contribute to the ionization and further destruction of PAHs. Overall, different Seyferts, even different regions in the same galaxy, e.g., those in NGC 3081, can contain PAH populations of different properties. Specifically, Seyferts that exhibit similar PAH characteristics to ESO137-G034 and MCG-05-23-016 also tend to have similar emission-line properties to them, suggesting that the explanations for PAH characteristics of ESO137-G034 and MCG-05-23-016 may also apply generally. These results have promising application in the era of JWST, especially in diagnosing different (i.e., radiative and kinetic) AGN feedback modes.

astro-ph.GA
2041-8205
Zhang, Lulu
f2f69a6d-9c10-40b8-a66e-0e0a73759f76
García-Bernete, Ismael
32d4c248-70e2-4ae9-8d43-07c62c2c94c9
Packham, Chris
0c83eff2-c7e9-4814-a0f3-ad73ec5c149b
Donnan, Fergus R.
dc210a4f-9244-4144-b188-72e5ef696d01
Rigopoulou, Dimitra
6ca651ec-f156-4b38-a899-1bfc9448b147
Hicks, Erin K.S.
ded5dc5d-5c31-46b4-80c6-c6f798a22f7f
Davies, Ric I.
49829114-3931-43c0-8d8b-4400fd027294
Shimizu, Taro T.
3b63b046-efd3-41ed-92cc-13c5bd042455
Alonso-Herrero, Almudena
8672ba48-8f27-45f2-a89f-2c62f8e34261
Almeida, Cristina Ramos
407b9f57-0072-415e-826d-7f711fc5fe65
Pereira-Santaella, Miguel
fb5125cd-2c04-4d71-8f14-d0669c6b4f1d
Ricci, Claudio
47c48bd5-233e-41dd-824a-3df26357d84f
Bunker, Andrew J.
4f9ebf02-2ab1-4684-9a21-f3ab19a23a99
Leist, Mason T.
392aaccf-0a64-42cd-9be1-d394727419cd
Rosario, David J.
d1194be4-0304-49ab-b2a7-293c75aa1550
García-Burillo, Santiago
48a403d9-b21b-4e63-8872-8fe043e213a6
Muñoz, Laura Hermosa
71037268-3587-42a4-909b-886fab697a7d
Combes, Francoise
2a323e9d-35ea-400f-97be-448c28897de4
Imanishi, Masatoshi
f74c529e-98a7-4367-875f-053e58922144
Labiano, Alvaro
3432edd0-d265-4c53-a421-32ace0349032
Esparza-Arredondo, Donaji
2d7063c2-fb23-4a43-b649-ca02a976e352
Bellocchi, Enrica
4545142e-9f61-4485-b676-fc0679682a17
Audibert, Anelise
a24a8f1c-422b-4f14-afa9-adcc8f864bdf
Fuller, Lindsay
7921782f-2fb0-4908-b388-28b0fc2956a6
González-Martín, Omaira
9d84142f-c1c3-4d3d-aaf6-ce241e356335
Hönig, Sebastian
be0bb8bc-bdac-4442-8edc-f735834f3917
Izumi, Takuma
cf268824-fda0-45c4-ae37-0a51e510a851
Levenson, Nancy A.
57c66b17-cc66-4e9e-8251-19132426cf57
López-Rodríguez, Enrique
ab531f9f-6bfa-4472-9d6c-cfa9dc81943d
Rouan, Daniel
e8e1299c-9a83-414e-bdd7-f48ccbfbe346
Stalevski, Marko
6f6b37b3-7a57-4024-b190-a2ea2d538051
Ward, Martin J.
563f4fe6-a983-42a1-9372-1e666c068160
et al.
Zhang, Lulu
f2f69a6d-9c10-40b8-a66e-0e0a73759f76
García-Bernete, Ismael
32d4c248-70e2-4ae9-8d43-07c62c2c94c9
Packham, Chris
0c83eff2-c7e9-4814-a0f3-ad73ec5c149b
Donnan, Fergus R.
dc210a4f-9244-4144-b188-72e5ef696d01
Rigopoulou, Dimitra
6ca651ec-f156-4b38-a899-1bfc9448b147
Hicks, Erin K.S.
ded5dc5d-5c31-46b4-80c6-c6f798a22f7f
Davies, Ric I.
49829114-3931-43c0-8d8b-4400fd027294
Shimizu, Taro T.
3b63b046-efd3-41ed-92cc-13c5bd042455
Alonso-Herrero, Almudena
8672ba48-8f27-45f2-a89f-2c62f8e34261
Almeida, Cristina Ramos
407b9f57-0072-415e-826d-7f711fc5fe65
Pereira-Santaella, Miguel
fb5125cd-2c04-4d71-8f14-d0669c6b4f1d
Ricci, Claudio
47c48bd5-233e-41dd-824a-3df26357d84f
Bunker, Andrew J.
4f9ebf02-2ab1-4684-9a21-f3ab19a23a99
Leist, Mason T.
392aaccf-0a64-42cd-9be1-d394727419cd
Rosario, David J.
d1194be4-0304-49ab-b2a7-293c75aa1550
García-Burillo, Santiago
48a403d9-b21b-4e63-8872-8fe043e213a6
Muñoz, Laura Hermosa
71037268-3587-42a4-909b-886fab697a7d
Combes, Francoise
2a323e9d-35ea-400f-97be-448c28897de4
Imanishi, Masatoshi
f74c529e-98a7-4367-875f-053e58922144
Labiano, Alvaro
3432edd0-d265-4c53-a421-32ace0349032
Esparza-Arredondo, Donaji
2d7063c2-fb23-4a43-b649-ca02a976e352
Bellocchi, Enrica
4545142e-9f61-4485-b676-fc0679682a17
Audibert, Anelise
a24a8f1c-422b-4f14-afa9-adcc8f864bdf
Fuller, Lindsay
7921782f-2fb0-4908-b388-28b0fc2956a6
González-Martín, Omaira
9d84142f-c1c3-4d3d-aaf6-ce241e356335
Hönig, Sebastian
be0bb8bc-bdac-4442-8edc-f735834f3917
Izumi, Takuma
cf268824-fda0-45c4-ae37-0a51e510a851
Levenson, Nancy A.
57c66b17-cc66-4e9e-8251-19132426cf57
López-Rodríguez, Enrique
ab531f9f-6bfa-4472-9d6c-cfa9dc81943d
Rouan, Daniel
e8e1299c-9a83-414e-bdd7-f48ccbfbe346
Stalevski, Marko
6f6b37b3-7a57-4024-b190-a2ea2d538051
Ward, Martin J.
563f4fe6-a983-42a1-9372-1e666c068160

Zhang, Lulu, García-Bernete, Ismael and Packham, Chris , et al. (2024) Polycyclic aromatic hydrocarbon emission in the central regions of three Seyferts and the implication for underlying feedback mechanisms. The Astrophysical Journal Letters, 975 (1), [L2]. (doi:10.3847/2041-8213/ad81d0).

Record type: Article

Abstract

We analyze JWST Mid-Infrared Instrument/Medium Resolution Spectrograph integral field unit observations of three Seyferts from the Galactic Activity, Torus, and Outflow Survey (GATOS) and showcase the intriguing polycyclic aromatic hydrocarbon (PAH) and emission-line characteristics in regions of ∼500 pc scales over or around their active galactic nuclei (AGN). Combing the measurements and model predictions, we find that the central regions containing a high fraction of neutral PAHs with small sizes, e.g., those in ESO137-G034, are in highly heated environments, due to collisional shock heating, with hard and moderately intense radiation fields. Such environments are proposed to result in inhibited growth or preferential erosion of PAHs, decreasing their average size and overall abundance. We additionally find that the central regions containing a high fraction of ionized PAHs with large sizes, e.g., those in MCG-05-23-016, are likely experiencing severe photoionization because of the radiative effects from the radiative shock precursor besides the AGN. The severe photoionization can contribute to the ionization and further destruction of PAHs. Overall, different Seyferts, even different regions in the same galaxy, e.g., those in NGC 3081, can contain PAH populations of different properties. Specifically, Seyferts that exhibit similar PAH characteristics to ESO137-G034 and MCG-05-23-016 also tend to have similar emission-line properties to them, suggesting that the explanations for PAH characteristics of ESO137-G034 and MCG-05-23-016 may also apply generally. These results have promising application in the era of JWST, especially in diagnosing different (i.e., radiative and kinetic) AGN feedback modes.

Text
2409.09772v2 - Author's Original
Available under License Creative Commons Attribution.
Download (7MB)
Text
Zhang_2024_ApJL_975_L2 - Version of Record
Available under License Creative Commons Attribution.
Download (11MB)

More information

Accepted/In Press date: 26 September 2024
Published date: 21 October 2024
Keywords: astro-ph.GA

Identifiers

Local EPrints ID: 496219
URI: http://eprints.soton.ac.uk/id/eprint/496219
ISSN: 2041-8205
PURE UUID: 45dff95f-563e-43e2-9354-e80ddc2ee3cf

Catalogue record

Date deposited: 09 Dec 2024 17:36
Last modified: 21 Aug 2025 03:01

Export record

Altmetrics

Contributors

Author: Lulu Zhang
Author: Ismael García-Bernete
Author: Chris Packham
Author: Fergus R. Donnan
Author: Dimitra Rigopoulou
Author: Erin K.S. Hicks
Author: Ric I. Davies
Author: Taro T. Shimizu
Author: Almudena Alonso-Herrero
Author: Cristina Ramos Almeida
Author: Miguel Pereira-Santaella
Author: Claudio Ricci
Author: Andrew J. Bunker
Author: Mason T. Leist
Author: David J. Rosario
Author: Santiago García-Burillo
Author: Laura Hermosa Muñoz
Author: Francoise Combes
Author: Masatoshi Imanishi
Author: Alvaro Labiano
Author: Donaji Esparza-Arredondo
Author: Enrica Bellocchi
Author: Anelise Audibert
Author: Lindsay Fuller
Author: Omaira González-Martín
Author: Takuma Izumi
Author: Nancy A. Levenson
Author: Enrique López-Rodríguez
Author: Daniel Rouan
Author: Marko Stalevski
Author: Martin J. Ward
Corporate Author: et al.

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×